The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light

We present a comparison of the SCUBA half degree extragalactic survey (SHADES) at 450 μm, 850 μm and 1100 μm with deep guaranteed time 15 μm AKARI FU-HYU survey data and Spitzer guaranteed time data at 3.6-24 μm in the Lockman hole east. The AKARI data was analysed using bespoke software based in pa...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2010-05, Vol.514, p.A10
Hauptverfasser: Serjeant, S., Negrello, M., Pearson, C., Mortier, A., Austermann, J., Aretxaga, I., Clements, D., Chapman, S., Dye, S., Dunlop, J., Dunne, L., Farrah, D., Hughes, D., Lee, H.-M., Matsuhara, H., Ibar, E., Im, M., Jeong, W.-S., Kim, S., Oyabu, S., Takagi, T., Wada, T., Wilson, G., Vaccari, M., Yun, M.
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Sprache:eng
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Zusammenfassung:We present a comparison of the SCUBA half degree extragalactic survey (SHADES) at 450 μm, 850 μm and 1100 μm with deep guaranteed time 15 μm AKARI FU-HYU survey data and Spitzer guaranteed time data at 3.6-24 μm in the Lockman hole east. The AKARI data was analysed using bespoke software based in part on the drizzling and minimum-variance matched filtering developed for SHADES, and was cross-calibrated against ISO fluxes. Our stacking analyses find AKARI 15 μm galaxies with $\ga$200 μJy contribute >10% of the 450 μm background, but only 0.3.
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/200913483